Ars Technica: The Moon’s gravitational pull on Earth, as evidenced by the oceans’ tides, has long been recognized; however, Earth also exerts a reciprocal pull on the Moon. That pull creates seismic waves, which must dissipate in the Moon’s interior. Scientists have attempted to calculate the effects of Earth’s tidal forces on the Moon, but until recently none of the calculations had proven satisfactory. In a new study published in Nature Geoscience, researchers propose that the Moon has a zone of low viscosity located at its core–mantle boundary. That partially melted zone helps dissipate the heat created by the seismic-wave action. Although the model goes a long way toward matching simulations with observations, more refinements are needed, the scientists say. Their research could prove important to furthering our understanding of how planetary bodies formed.
The finding that the Saturnian moon may host layers of icy slush instead of a global ocean could change how planetary scientists think about other icy moons as well.
Modeling the shapes of tree branches, neurons, and blood vessels is a thorny problem, but researchers have just discovered that much of the math has already been done.
January 29, 2026 12:52 PM
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